Pages that link to "Item:Q2436497"
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The following pages link to Scenario of accelerating universe: role of phenomenological \(\varLambda\) models (Q2436497):
Displaying 9 items.
- Phenomenological fluids from interacting tachyonic scalar fields (Q458065) (← links)
- Scenario of inflationary cosmology from the phenomenological \(\Lambda \) models (Q735360) (← links)
- Time variable \(\Lambda \) and the accelerating universe (Q2429960) (← links)
- Phenomenology of \(\Lambda \)-CDM model: a possibility of accelerating universe with positive pressure (Q2429981) (← links)
- The dark clump near Abell 1942: dark matter halo or statistical fluke? (Q3408426) (← links)
- Phenomenological dark energy model with hybrid dynamic cosmological constant (Q5023556) (← links)
- A higher dimensional cosmological model for the search of dark energy source (Q6204307) (← links)
- Higher dimensional phantom dark energy model ending at a de-Sitter phase (Q6542197) (← links)
- Cosmological model with linear equation of state parameter in \(f((R, L_m)\) gravity (Q6649601) (← links)